      The Rindler metric describes the near horizon geometry of finite-temperature black hole. The ubiquity of the Rindler horizon could be not enough to determine a pole-skipping in the corresponding Green's functions. However we can use the near horizon analysis to obtain “special points” making the equation of motion have two incoming solutions. The Rindler metric is given as[1]}
\(ds^2=-K^2\rho ^2dt^2+d\rho ^2+\frac{1}{4K^2}dx^2+\frac{1}{4K^2}dy^2,\) 
